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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F14%3A00428328%21RIV15-AV0-67985815
rdf:type
n15:Vysledek skos:Concept
dcterms:description
The anisotropic nature of active galactic nuclei (AGN) is thought to be responsible for the observational differences between type-1 (pole-on) and type-2 (edge-on) nearby Seyfert-like galaxies. In this picture, the detection of emission and/or absorption features is directly correlated to the inclination of the system. The AGN structure can be further probed by using the geometry-sensitive technique of polarimetry, yet the pairing between observed polarization and Seyfert type remains poorly examined. Based on archival data, I report here the first compilation of 53 estimated AGN inclinations matched with ultraviolet/optical continuum polarization measurements. Corrections, based on the polarization of broad emission lines, are applied to the sample of Seyfert-2 AGN to remove dilution by starburst light and derive information about the scattered continuum alone. The resulting compendium agrees with past empirical results, i.e. type-1 AGN show low polarization degrees (P 1 per cent) predominantly associated with a polarization position angle parallel to the projected radio axis of the system, while type-2 objects show stronger polarization percentages (P > 7 per cent) with perpendicular polarization angles. The anisotropic nature of active galactic nuclei (AGN) is thought to be responsible for the observational differences between type-1 (pole-on) and type-2 (edge-on) nearby Seyfert-like galaxies. In this picture, the detection of emission and/or absorption features is directly correlated to the inclination of the system. The AGN structure can be further probed by using the geometry-sensitive technique of polarimetry, yet the pairing between observed polarization and Seyfert type remains poorly examined. Based on archival data, I report here the first compilation of 53 estimated AGN inclinations matched with ultraviolet/optical continuum polarization measurements. Corrections, based on the polarization of broad emission lines, are applied to the sample of Seyfert-2 AGN to remove dilution by starburst light and derive information about the scattered continuum alone. The resulting compendium agrees with past empirical results, i.e. type-1 AGN show low polarization degrees (P 1 per cent) predominantly associated with a polarization position angle parallel to the projected radio axis of the system, while type-2 objects show stronger polarization percentages (P > 7 per cent) with perpendicular polarization angles.
dcterms:title
A Compendium of AGN inclinations with corresponding UV/optical continuum polarization measurements A Compendium of AGN inclinations with corresponding UV/optical continuum polarization measurements
skos:prefLabel
A Compendium of AGN inclinations with corresponding UV/optical continuum polarization measurements A Compendium of AGN inclinations with corresponding UV/optical continuum polarization measurements
skos:notation
RIV/67985815:_____/14:00428328!RIV15-AV0-67985815
n4:aktivita
n5:I
n4:aktivity
I
n4:cisloPeriodika
1
n4:dodaniDat
n7:2015
n4:domaciTvurceVysledku
Marin, Frederic
n4:druhVysledku
n16:J
n4:duvernostUdaju
n10:S
n4:entitaPredkladatele
n13:predkladatel
n4:idSjednocenehoVysledku
634
n4:idVysledku
RIV/67985815:_____/14:00428328
n4:jazykVysledku
n11:eng
n4:klicovaSlova
polarization; active galacticnuclei; radiative transfer
n4:klicoveSlovo
n8:active%20galacticnuclei n8:polarization n8:radiative%20transfer
n4:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n4:kontrolniKodProRIV
[27EC5C36491F]
n4:nazevZdroje
Monthly Notices of the Royal Astronomical Society
n4:obor
n6:BN
n4:pocetDomacichTvurcuVysledku
1
n4:pocetTvurcuVysledku
1
n4:rokUplatneniVysledku
n7:2014
n4:svazekPeriodika
441
n4:tvurceVysledku
Marin, Frederic
n4:wos
000336249300039
s:issn
0035-8711
s:numberOfPages
14
n14:doi
10.1093/mnras/stu593